Space Weather Conditions at the Time of the Galaxy 15 Anomaly NOAA Tiger Team • W. F. Denig (NGDC) • J. C. Green (SWPC, now NGDC) • D. C. Wilkinson (NGDC) • J. V. Rodriguez (CIRES @ SWPC) • H. J. Singer (SWPC) • P. T. Loto'aniu (CIRES @ SWPC) • D. A. Biesecker (SWPC) • W. Murtagh (SWPC) Galaxy 15 Satellite Presented at the Photo Credit: Orbital Sciences 2011 Space Weather Workshop 26-29 April 2011 Boulder, CO OUTLINE Space Weather Conditions – 05 Apr 10 Space Weather describes changes in the interconnected system from the Sun to Earth This presentation follows space weather conditions progressing from the sun to near the Galaxy 15 location showing: 1. Events that occurred at the sun 2. Resulting global changes in the near-earth space environment 3. Local changes near Galaxy 15 in the energetic charged particles that can cause satellite charging and electronic component failure Summary Solar activity was elevated but not remarkable Global geomagnetic activity described by the AL auroral electrojet index and Kp were extreme. Other SWx indices were more moderate Local measurements near Galaxy 15 show that a large geomagnetic substorm occurred 48 minutes prior to the anomaly. The substorm caused remarkable increases in the measured local flux of energetic particles known to cause surface or internal satellite charging 3 Background (1 of 2) Galaxy 15 Satellite Anomaly - Impacts 08 Apr 2010 – Intelsat reports that the Galaxy 15 stopped responding to ground commands (Anomaly time: 05 April @ 09:48 UTC) 10 Apr 2010 – FAA predicts erosion of WAAS capability due to Galaxy 15 failure 20 Apr 2010 – Orbital attributes the loss of Galaxy 15 to space weather 30 Apr 2010 – Intel reports Galaxy 15 still adrift and threatens nearby satellites (i.e. frequency interference) 4 Background (2 of 2) Operational Timeline Operational Timeline – Universal Time (UT) April 3, 2010 09:54 B7 solar flare (sunspot region 1059) 10:33 CME first visible 22:04 SWPC Daily Forecast issued – Notes Flare and Coronal Mass Ejection (CME) – Geomagnetic quiet expected: 04-05 April April 4 22:01 Daily Forecast issued (left text) – Flank of CME may contribute to elevated activity on April 7 April 5 05:33 Warning issued: K=4 05:44 Alert issued: K=4 08:04 Warning issued – Sudden Impulse (CME hits ACE @ 07:56 UT) 09:16 Warning issued: K=5 09:17 Alert issued: K=5 09:22 Alert issued: K=6 09:48 Galaxy 15 anomaly 09:56 Alert issued: K=7 SWW – 26-29 April 2011 5 Space Weather Conditions 1. Events at the Sun (1 of 2) Solar activity prior to the Galaxy 15 anomaly on April 05 at 9:48 was elevated but unremarkable. On 03 April @ 9:54 UT (2 days prior to the anomaly) a solar B7 flare was observed by the NOAA GOES-14 X-Ray Sensor (XRS) – Flares of this intensity are not usually associated with intense space weather – In solar cycle 23 there were >14,000 flares more intense than a B7-level flare – There have already been 278 flares more intense than B7 in the new cycle – Source of the flare was decaying active region 1059 (S22W15) with 4 sunspots Satellite Eclipse B7 FLARE 6 Space Weather Conditions 1. Events at the Sun (2 of 2) April 03 @ 10:33 UT ~30 minutes after the flare an earthward SOHO/LASCO directed coronal mass ejection (CME) was observed – SOHO/LASCO imager showed a modest partial Halo event – Side view of the CME from the NASA STEREO COR2 instrument indicated that it was moving southward and only the ‘edge’ would graze earth – Measured plane of sky speed was 512 km/s – Moderate speeds and ‘edge’ impacts such as these typically cause weaker, shorter duration geomagnetic storms NASA/ESA – Solar cycle 23 had ~500 faster Earth directed CME’s STEREO COR2 This event was classified as a moderate CME ejected from an otherwise quiet sun – F10.7 was 77 sfu, the sunspot number was 27 and the x-ray background was a modest 3.9x10-8 Watts m-2 EARTH – At solar maximum, F10.7 is expected to be about 150 sfu and the sunspot number to be at least 3x greater NASA 7 Space Weather Conditions 2. Global Environment At Earth (1 of 2) Galaxy 15 anomaly April 05 07:56 UT – Nearly 2 days CME detected after the CME lifted off from the by ACE sun, it was observed by the NASA ACE satellite upstream of earth – It takes ~30 minutes for the solar wind to propagate from ACE to Earth – The solar wind magnetic field turned southward (negative) – The solar wind speed increased from ~500 to >700 km/s Such solar wind conditions often result in a moderate geomagnetic storm Note: ACE is the NASA Advanced Composition Explorer located in a halo orbit near the L1 sun-earth Lagrangian point approximately ~1.5x106 km in the sunward direction. Plot shows solar wind parameters Data Source: NASA Omni observed at ACE, time-shifted to Earth. 8 Space Weather Conditions 2. Global Environment At Earth (2 of 2) Some (but not all) global geomagnetic activity indicators were extreme immediately prior to the anomaly 01 Oct 05 to 01 May 10 Currently only quick look plots are available for April AL index was <-2000 nT prior to the anomaly. Larger values observed only once previously during Galaxy 15 lifetime (launched: 13 Oct 05) Kp index reached 7.7 prior to the anomaly – larger values were observed only once previously during the Galaxy 15 lifetime ? However, Dst index reached -32 nT prior to anomaly indicating only a moderate storm – similar to many previously observed levels during the Galaxy 15 lifetime Data Source: Kyoto World Data Center & German Research Centre for Geosciences 9 Space Weather Conditions 3. Local Environment At Galaxy 15 (1 of 4) April 05 @ 09:00 UT: GOES magnetometers and particle instruments showed a major reconfiguration of the magnetosphere indicative of a substorm and injection of energetic particles into the nightside, geosynchronous orbit location Galaxy 15 (133 W) Anomaly 09:48 UT Satellite Locations Eclipse 10 Space Weather Conditions 3. Local Environment At Galaxy 15 (2 of 4) Surface Charging: Electron Environment (Low-to-Medium Energy Electrons) April 05 @ 9:00 – 48 minute prior to the Galaxy 15 anomaly the 40-to-475 keV electron flux increased at GOES 14 and 15 – 75-to-475 keV electron flux was the highest observed since GOES 14 was turned on in July 2009 and since GOES 15 was turned on in April 2010 – High electron fluxes are notable although surface charging potentials cannot be accurately estimated without lower energy (<40 keV) particle measurements and detailed modeling of their interactions with specific satellite surface materials Galaxy 15 anomaly GOES 14 ----- Satellite Locations GOES 15 ----- Note: Multiple curves for each GOES satellite correspond to different telescope “look” directions 11
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